logo
Milky Way has 50-50 chance of colliding with neighbor galaxy

Milky Way has 50-50 chance of colliding with neighbor galaxy

The Hill06-06-2025
The collision of the Milky Way and Andromeda galaxies that scientists believed was inevitable has a much lower probability than previously thought.
The Associated Press reported Monday that astronomers in Finland have determined that our galaxy has a 50-50 chance of colliding with the neighboring Andromeda within the next 10 billion years. The previous theory suggested that the two galaxies had a high probability of colliding within the next five billion years.
'Based on the best available data, the fate of our galaxy is still completely open,' the team wrote in the study, which appeared in Nature Astronomy.
A team led by University of Helsinki researcher Till Sawala simulated all possible scenarios using the latest data from NASA's Hubble Space Telescope and the European Space Agency's Gaia star-tracking mission. According to Space.com, the simulation yielded some surprising results.
'A head-on collision is very unlikely, we found a less than 2 percent chance for that,' Sawala said. 'In most of the cases that lead to a merger, the two galaxies will indeed fly past each other at first, which will lead to a loss of orbital energy, and subsequently to a merger.
'How close they come on their first passage is very uncertain, however, and if they don't come very close, meaning if their distance is more than around 500,000 light-years, they might not merge at all,' the researcher added.
Sawala said he was not prepared for what his team found.
'In short, the probability went from near-certainty to a coin flip,' Sawala noted.
The study relied on newer and more precise information, and the team took into consideration a 'more complete system,' including the potential effects of the Large Magellanic Cloud. The dwarf galaxy is the Milky Way's largest satellite galaxy, Space.com reported.
Ultimately, the astronomers found that the Milky Way and Andromeda would inevitably collide if the two galaxies' orbits come close enough to affect a gravitational pull on one another. If they stay well separated, the merger won't happen.
While the scenarios indicated a less likely merger between the two, they found that the Milky Way is far more likely to cannibalize the Large Magellanic Cloud.
The research indicates that this newly theorized merger is likely to happen over the next two billion years.
Orange background

Try Our AI Features

Explore what Daily8 AI can do for you:

Comments

No comments yet...

Related Articles

First-ever evidence of star 'double detonation' captured in stunning image
First-ever evidence of star 'double detonation' captured in stunning image

Yahoo

time37 minutes ago

  • Yahoo

First-ever evidence of star 'double detonation' captured in stunning image

When you buy through links on our articles, Future and its syndication partners may earn a commission. For the first time, astronomers have captured stunning visual evidence of a star double-detonating itself to death. The twin eruption was discovered by scientists studying two concentric rings of calcium that surround SNR 0509-67.5, a remnant of a star that met its explosive demise in a type Ia supernova centuries ago. And the discovery isn't just a pretty picture. The researchers who made it say that much of our knowledge of how the universe expands — a major controversy in cosmology — depends on reliably measuring this type of supernova, which is also the primary source of iron throughout the cosmos. The scientists published their findings July 2 in the journal Nature Astronomy. For these reasons, "the explosions of white dwarfs play a crucial role in astronomy," study first author Priyam Das, a graduate student at the University of New South Wales Canberra in Australia, said in a statement. "Yet, despite their importance, the long-standing puzzle of the exact mechanism triggering their explosion remains unsolved." Type Ia supernovas occur when the material from one star is stolen by the husk of a co-orbiting dead star, known as a white dwarf, leading to a gigantic thermonuclear explosion. Yet not all the ways that white dwarves detonate are accounted for. Astronomers assume that these white dwarves steadily snatch their neighboring star's material, accumulating it until they reach a critical mass — the Chandrasekhar limit — and explode. But astronomers have found hints suggesting that this isn't the only way the husks blow up. Related: Supernova that lit up Earth's skies 843 years ago has a flowering 'zombie star' at its heart — and it's still exploding To search for direct evidence of a different ype of detonation, the researchers pointed the European Southern Observatory's Very Large Telescope at SNR 0509-67.5, a supernova that displays a clear shock wave shell pattern. Using the telescope's Multi Unit Spectroscopic Explorer instrument, they found two separate rings of calcium surrounding the remnants of the explosion. This is "a clear indication that white dwarfs can explode well before they reach the famous Chandrasekhar mass limit, and that the 'double-detonation' mechanism does indeed occur in nature," second-author Ivo Seitenzahl, a nuclear astrophysicist at the University of New South Wales Canberra, said in the statement. RELATED STORIES —Rare quadruple supernova on our 'cosmic doorstep' will shine brighter than the moon when it blows up in 23 billion years —Weird repeating explosion beyond the Milky Way is one of the hottest blasts scientists have ever seen —A nearby supernova nearly blew our solar system to bits 4 billion years ago, new research suggests The researchers propose that this white dwarf exploded by blanketing itself in stolen helium from its neighbor that then ignited, sending a shockwave inwards that caused the dead star's core to blow in a second, larger, explosion. Studying this dual detonation could have important implications for our wider understanding of the universe. No matter which way they occur, type Ia supernovas are thought to always explode with the same brightness, making them "standard candles" from which astronomers can measure far-off distances and calculate the expansion rate of our universe. In recent years, contesting measurements of this expansion rate, known as the Hubble constant, have sparked a major crisis in cosmology. "This tangible evidence of a double-detonation not only contributes towards solving a long-standing mystery, but also offers a visual spectacle," Das said. "Revealing the inner workings of such a spectacular cosmic explosion is incredibly rewarding."

See Mercury at greatest elongation, its farthest from the sun in the evening sky this week
See Mercury at greatest elongation, its farthest from the sun in the evening sky this week

Yahoo

time16 hours ago

  • Yahoo

See Mercury at greatest elongation, its farthest from the sun in the evening sky this week

When you buy through links on our articles, Future and its syndication partners may earn a commission. Mercury reaches its point of greatest eastern elongation on Friday (July 4), presenting an excellent opportunity to spot the rocky planet during its evening apparition in the post-sunset sky. Astronomers describe Mercury as an "inferior planet", because its orbital path around the sun is much closer than that of Earth. As a result, Mercury never strays far from the sun in our sky and always appears low on the horizon compared to planets like Jupiter and Mars, whose distant orbits allow them to ride high on the line of the ecliptic (the plane of the major planets' path around the sun). The point at which Mercury appears most distant from the sun in Earth's sky, known as its point of greatest elongation, will occur at 00:37 a.m. EDT (0437 GMT) on July 4, according to stargazing website Viewers in the U.S. will have a golden opportunity to spot Mercury shining low above the western horizon immediately after sunset over the coming days. The rocky world will appear as a bright "evening star" approximately 15 degrees above the western horizon in the constellation Cancer at sunset for viewers in New York on July 4. For context, 10 degrees is roughly the same as the span of your clenched fist when held at arms length against the night sky. Mercury's low altitude could make it a challenging target for those in built-up areas, so we would advise scoping out a spot with a clear horizon ahead of time if you want to catch a glimpse of the fleet-footed planet before it sets less than an hour and a half after sundown. The "Great Bear" of the constellation Ursa Major will become visible around the time Mercury slips out of view, with the stars of Leo and the red light of Mars beating a path toward the western horizon as the night wears on. TOP TELESCOPE PICK Want to see Mercury, Mars, and Regulus all in the night sky? The Celestron NexStar 4SE is ideal for beginners wanting quality, reliable and quick views of celestial objects. For a more in-depth look at our Celestron NexStar 4SE review. Stargazers hoping to explore the wonders of the cosmos for themselves should check out our roundup of the best telescopes and binoculars available in 2025. If you're new to the hobby you should also check out our roundup of the top paid and free smartphone astronomy apps, many of which use augmented reality tech to help you find your way around the night sky. Editor's Note: If you snap a picture of Mercury and want to share it with readers, then please send it alongside your comments, name and location to spacephotos@

Hubble Telescope finds stellar nursery in Taurus Molecular Cloud
Hubble Telescope finds stellar nursery in Taurus Molecular Cloud

Yahoo

timea day ago

  • Yahoo

Hubble Telescope finds stellar nursery in Taurus Molecular Cloud

When you buy through links on our articles, Future and its syndication partners may earn a commission. The Hubble Space Telescope searches the universe to understand how planets, stars, and galaxies form. Recently, it captured this image of a nebula known as GN 04.32.8 within a larger stellar nursery called the Taurus Molecular Cloud. According to the European Space Agency (ESA), the GN 04.32.8 nebula is classified as a reflection nebula, as it does not emit its own light, but instead its clouds of space dust reflect the light of nearby stars. The reflection nebula is more brightly illuminated around three young bright stars, the centermost being star V1025 Tauri. This star is a variable star, meaning that it's very chaotic and active as it's beginning its stellar evolution. The Taurus Molecular Cloud, where GN 04.32.8 lies, is in the constellation Taurus, around 480 light-years from Earth. The Taurus Molecular Cloud is one of the closest and most well-known stellar nurseries, making it an easy place to study how stars are born and evolve. But it's not the only thing in this picture that's newly formed. Lower down in this image is a small squished orange spot with a dark line through it. It's easy to miss but important to study, as it's a newly formed protostar surrounded by a protoplanetary disk. Because the disk is edge-on to the Hubble Space Telescope, astronomers can zoom in to further study how this disk formed, revealing more about the early universe. You can read more about baby stars and the Hubble Space Telescope's photographs as astronomers continue peering deep into our universe.

DOWNLOAD THE APP

Get Started Now: Download the App

Ready to dive into a world of global content with local flavor? Download Daily8 app today from your preferred app store and start exploring.
app-storeplay-store